Zobrazeno 1 - 10
of 1 128
pro vyhledávání: '"Kleimann A"'
Autor:
Eugenie Werbenko, David J. J. de Gorter, Simon Kleimann, Denise Beckmann, Vanessa Waltereit-Kracke, Julia Reinhardt, Fabienne Geers, Peter Paruzel, Uwe Hansen, Thomas Pap, Theresia E. B. Stradal, Berno Dankbar
Publikováno v:
Scientific Reports, Vol 14, Iss 1, Pp 1-13 (2024)
Abstract Bone resorption is highly dependent on the dynamic rearrangement of the osteoclast actin cytoskeleton to allow formation of actin rings and a functional ruffled border. Hem1 is a hematopoietic-specific subunit of the WAVE-complex which regul
Externí odkaz:
https://doaj.org/article/7158c6618faa4174a45185de02e0dde3
Autor:
Fraternale, Federico, Adhikari, Laxman, Fichtner, Horst, Kim, Tae K., Kleimann, Jens, Oughton, Sean, Pogorelov, Nikolai V., Roytershteyn, Vadim, Smith, Charles W., Usmanov, Arcadi V., Zank, G P., Zhao, Lingling
The solar wind (SW) and local interstellar medium (LISM) are turbulent media. Their interaction is governed by complex physical processes and creates heliospheric regions with significantly different properties in terms of particle populations, bulk
Externí odkaz:
http://arxiv.org/abs/2207.14115
Autor:
Kleimann, Jens, Röken, Christian
Rotationally symmetric bodies with longitudinal cross sections of parabolic shape are frequently used to model astrophysical objects, such as magnetospheres and other blunt objects, immersed in interplanetary or interstellar gas or plasma flows. We d
Externí odkaz:
http://arxiv.org/abs/2207.07419
Publikováno v:
A&A 663, A10 (2022)
Context. State of the art simulations of astrospheres are modelled using three-dimensional (3D) magnetohydrodynamics (MHD). An astrospheric interaction of a stellar wind (SW) with its surrounding interstellar medium (ISM) can only generate a bow shoc
Externí odkaz:
http://arxiv.org/abs/2205.04823
Autor:
Kleimann, Martin, Schmerer, Hans-Jörg
Publikováno v:
In Transportation Research Part D June 2024 131
We derive an exact, time-dependent analytical magnetic field solution for the inner heliosheath, which satisfies both the induction equation of ideal magnetohydrodynamics in the limit of infinite electric conductivity and the magnetic divergence cons
Externí odkaz:
http://arxiv.org/abs/2110.12893
Autor:
Beterams, A., Püning, C., Wyink, B., Grosse-Kleimann, J., Gölz, G., Schönknecht, A., Alter, T., Reich, F.
Publikováno v:
In International Journal of Food Microbiology 2 April 2024 414
Autor:
Baalmann, Lennart R., Scherer, Klaus, Kleimann, Jens, Fichtner, Horst, Bomans, Dominik J., Weis, Kerstin
Publikováno v:
A&A 650, A36 (2021)
Context. While the shapes of many observed bow shocks can be reproduced by simple astrosphere models, more elaborate approaches have recently been used to explain differing observable structures. Aims. By placing perturbations of an otherwise homogen
Externí odkaz:
http://arxiv.org/abs/2104.03748
Publikováno v:
In Meat Science February 2024 208
Autor:
Fichtner, Horst, Kleimann, Jens, Yoon, Peter H., Scherer, Klaus, Oughton, Sean, Engelbrecht, N. Eugene
Publikováno v:
The Astrophysical Journal, Volume 901, Issue 1, id.76, 7 pp., 2020
Measurements made with the Voyager 1 spacecraft indicate that significant levels of compressive fluctuations exist in the inner heliosheath. Some studies have already been performed with respect to the mirror-mode instability in the downstream region
Externí odkaz:
http://arxiv.org/abs/2010.04264